Inflating magnetically charged braneworlds

被引:14
|
作者
Cho, I
Vilenkin, A
机构
[1] Univ Paris 11, Phys Theor Lab, F-91405 Orsay, France
[2] Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
来源
PHYSICAL REVIEW D | 2004年 / 69卷 / 04期
关键词
D O I
10.1103/PhysRevD.69.045005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Numerical solutions of Einstein, scalar, and gauge field equations are found for static and inflating defects in a higher-dimensional spacetime. The defects have (3+1)-dimensional core and magnetic monopole configuration in n=3 extra dimensions. For the symmetry-breaking scale eta below the critical value eta(c), the defects are characterized by a flat worldsheet geometry and asymptotically flat extra dimensions. The critical scale eta(c) is comparable to the higher-dimensional Planck scale and has some dependence on the gauge and scalar couplings. For eta=eta(c), the extra dimensions degenerate into a "cigar," and for eta>eta(c) all static solutions are singular. The singularity can be removed if the requirement of staticity is relaxed and defect cores are allowed to inflate. The inflating solutions have de Sitter worldsheets and cigar geometry in the extra dimensions. Exact analytic solutions describing the asymptotic behavior of these inflating monopoles are found and the parameter space of these solutions is analyzed.
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页数:15
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